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Reconstruction of the magnetotail current sheet structure using multi-point Cluster measurements. / Runov, A.; Sergeev, V. A.; Nakamura, R.; Baumjohann, W.; Zhang, T. L.; Asano, Y.; Volwerk, M.; Vörös, Z.; Balogh, A.; R̀me, H.

In: Planetary and Space Science, Vol. 53, No. 1-3, 2005, p. 237-243.

Research output: Contribution to journalArticlepeer-review

Harvard

Runov, A, Sergeev, VA, Nakamura, R, Baumjohann, W, Zhang, TL, Asano, Y, Volwerk, M, Vörös, Z, Balogh, A & R̀me, H 2005, 'Reconstruction of the magnetotail current sheet structure using multi-point Cluster measurements', Planetary and Space Science, vol. 53, no. 1-3, pp. 237-243. https://doi.org/10.1016/j.pss.2004.09.049

APA

Runov, A., Sergeev, V. A., Nakamura, R., Baumjohann, W., Zhang, T. L., Asano, Y., Volwerk, M., Vörös, Z., Balogh, A., & R̀me, H. (2005). Reconstruction of the magnetotail current sheet structure using multi-point Cluster measurements. Planetary and Space Science, 53(1-3), 237-243. https://doi.org/10.1016/j.pss.2004.09.049

Vancouver

Runov A, Sergeev VA, Nakamura R, Baumjohann W, Zhang TL, Asano Y et al. Reconstruction of the magnetotail current sheet structure using multi-point Cluster measurements. Planetary and Space Science. 2005;53(1-3):237-243. https://doi.org/10.1016/j.pss.2004.09.049

Author

Runov, A. ; Sergeev, V. A. ; Nakamura, R. ; Baumjohann, W. ; Zhang, T. L. ; Asano, Y. ; Volwerk, M. ; Vörös, Z. ; Balogh, A. ; R̀me, H. / Reconstruction of the magnetotail current sheet structure using multi-point Cluster measurements. In: Planetary and Space Science. 2005 ; Vol. 53, No. 1-3. pp. 237-243.

BibTeX

@article{8b0a404731894f23b9364b7074ed0a82,
title = "Reconstruction of the magnetotail current sheet structure using multi-point Cluster measurements",
abstract = "In this paper we analyze the vertical structure of the magnetotail current sheet for a few intervals during which Cluster repeatedly crosses the neutral sheet due to fast flapping motion. They include fast flows with episodes of flow reversals. The curl, gradient and divergence of the magnetic field are estimated using linear gradient/curl estimator techniques. The reconstruction of the electric current and magnetic field profiles are performed by integration of the estimated gradient scales. We found examples of thin current sheets, (half-thickness of 1000 km) with the current density maximum at the magnetic equator (Bx = 0), as well as examples of off-center or bifurcated current sheets.",
keywords = "Bursty bulk flow, Current sheet, Magnetospheric tail, Neutral sheet",
author = "A. Runov and Sergeev, {V. A.} and R. Nakamura and W. Baumjohann and Zhang, {T. L.} and Y. Asano and M. Volwerk and Z. V{\"o}r{\"o}s and A. Balogh and H. {\`R}me",
year = "2005",
doi = "10.1016/j.pss.2004.09.049",
language = "English",
volume = "53",
pages = "237--243",
journal = "Planetary and Space Science",
issn = "0032-0633",
publisher = "Elsevier",
number = "1-3",
note = "Conference on Magnetospheric Response to Solar Activity ; Conference date: 09-09-2003 Through 12-09-2003",

}

RIS

TY - JOUR

T1 - Reconstruction of the magnetotail current sheet structure using multi-point Cluster measurements

AU - Runov, A.

AU - Sergeev, V. A.

AU - Nakamura, R.

AU - Baumjohann, W.

AU - Zhang, T. L.

AU - Asano, Y.

AU - Volwerk, M.

AU - Vörös, Z.

AU - Balogh, A.

AU - R̀me, H.

PY - 2005

Y1 - 2005

N2 - In this paper we analyze the vertical structure of the magnetotail current sheet for a few intervals during which Cluster repeatedly crosses the neutral sheet due to fast flapping motion. They include fast flows with episodes of flow reversals. The curl, gradient and divergence of the magnetic field are estimated using linear gradient/curl estimator techniques. The reconstruction of the electric current and magnetic field profiles are performed by integration of the estimated gradient scales. We found examples of thin current sheets, (half-thickness of 1000 km) with the current density maximum at the magnetic equator (Bx = 0), as well as examples of off-center or bifurcated current sheets.

AB - In this paper we analyze the vertical structure of the magnetotail current sheet for a few intervals during which Cluster repeatedly crosses the neutral sheet due to fast flapping motion. They include fast flows with episodes of flow reversals. The curl, gradient and divergence of the magnetic field are estimated using linear gradient/curl estimator techniques. The reconstruction of the electric current and magnetic field profiles are performed by integration of the estimated gradient scales. We found examples of thin current sheets, (half-thickness of 1000 km) with the current density maximum at the magnetic equator (Bx = 0), as well as examples of off-center or bifurcated current sheets.

KW - Bursty bulk flow

KW - Current sheet

KW - Magnetospheric tail

KW - Neutral sheet

UR - http://www.scopus.com/inward/record.url?scp=19944428522&partnerID=8YFLogxK

U2 - 10.1016/j.pss.2004.09.049

DO - 10.1016/j.pss.2004.09.049

M3 - Article

VL - 53

SP - 237

EP - 243

JO - Planetary and Space Science

JF - Planetary and Space Science

SN - 0032-0633

IS - 1-3

T2 - Conference on Magnetospheric Response to Solar Activity

Y2 - 9 September 2003 through 12 September 2003

ER -

ID: 36754439